A | B |
Nuclear Fusion | nuclei of small atoms combine to form a different atom with the release of energy. |
Radiative Zone | surrounds the core where energy moves outward from atom to atom to form electromagnetic waves or radiation. |
Convective zone | surrounds the radiative zone area where energy is carried upward by movement of gases as hot gases rises and cool gases sinks. |
Photosphere | visible surface of the sun. |
Chromosphere | lies above the photosphere reddish in color due to hydrogen. |
Corona | outermost layer of the atmosphere. |
Core | center of the sun where nuclear fusion occurs fusion of hydrogen into helium 15 million degrees Celsius hottest area. |
Prominence | a loop of cooled gas that extends above the photosphere flow along magnetic curved lines from of one polarity to opposite polarity. |
Solar flare | an explosive release of energy. |
Aurora | interaction when solar wind reaches Earth's magnetosphere produced bands of colored lights. |
Solar Wind | electorally charged particles thrown off from the sun that travels outward in space. |
Coronal mass ejection | gas from the corona that is very violently ejected or thrown into space. |
E=mc2 | law of relativity |
E | equals energy |
m | equals mass or amount of matter used |
c | equals the speed of light |
convection | hot gas rise and cooler gas sinks |